A shared accretion instability for black holes and neutron stars
Artikel i vetenskaplig tidskrift, 2023

Accretion disks around compact objects are expected to enter an unstable phase at high luminosity1. One instability may occur when the radiation pressure generated by accretion modifies the disk viscosity, resulting in the cyclic depletion and refilling of the inner disk on short timescales2. Such a scenario, however, has only been quantitatively verified for a single stellar-mass black hole3-5. Although there are hints of these cycles in a few isolated cases6-10, their apparent absence in the variable emission of most bright accreting neutron stars and black holes has been a continuing puzzle11. Here we report the presence of the same multiwavelength instability around an accreting neutron star. Moreover, we show that the variability across the electromagnetic spectrum-from radio to X-ray-of both black holes and neutron stars at high accretion rates can be explained consistently if the accretion disks are unstable, producing relativistic ejections during transitions that deplete or refill the inner disk. Such a new association allows us to identify the main physical components responsible for the fast multiwavelength variability of highly accreting compact objects.

Författare

Federico M. Vincentelli

Villanova University

University of Southampton

Instituto de Astrofísica de Canarias

Universidad de la Laguna

Joseph Neilsen

Villanova University

Alexandra J. Tetarenko

Texas Tech University at Lubbock

Y. Cavecchi

Universitat Politecnica de Catalunya

Universidad Nacional Autónoma de México

N. Castro Segura

University of Southampton

Santiago Del Palacio

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

J. van den Eijnden

University of Oxford

G. Vasilopoulos

Yale University

Observatoire Astronomique de Strasbourg

D. Altamirano

University of Southampton

M. Armas Padilla

Universidad de la Laguna

Instituto de Astrofísica de Canarias

C. D. Bailyn

Yale University

Tomaso Belloni

Istituto nazionale di astrofisica (INAF)

D. J.K. Buisson

University of Southampton

V. A. Cúneo

Instituto de Astrofísica de Canarias

Universidad de la Laguna

N. Degenaar

Anton Pannekoek Institute for Astronomy

C. Knigge

University of Southampton

K. S. Long

Eureka Scientific

Space Telescope Science Institute (STScI)

F. Jiménez-Ibarra

Instituto de Astrofísica de Canarias

Universidad de la Laguna

J. Milburn

California Institute of Technology (Caltech)

T. Muñoz Darias

Instituto de Astrofísica de Canarias

Universidad de la Laguna

M. Özbey Arabacı

University of Southampton

R. Remillard

Massachusetts Institute of Technology (MIT)

T. Russell

Istituto nazionale di astrofisica (INAF)

Nature

0028-0836 (ISSN) 1476-4687 (eISSN)

Vol. 615 7950 45-49

Ämneskategorier

Acceleratorfysik och instrumentering

Astronomi, astrofysik och kosmologi

Fusion, plasma och rymdfysik

DOI

10.1038/s41586-022-05648-3

PubMed

36859580

Mer information

Senast uppdaterat

2023-09-15